Gravitation, electromagnetism and cosmological constant in purely affine gravity
Nikodem J. Poplawski

TL;DR
This paper explores a purely affine gravity formulation combining electromagnetism and the cosmological constant, revealing that simple additive models are invalid and suggesting more complex underlying affine Lagrangians.
Contribution
It demonstrates that the sum of affine Lagrangians for electromagnetism and the cosmological constant is not equivalent to their metric counterparts, indicating a need for more complex models.
Findings
Sum of affine Lagrangians is dynamically inequivalent to metric sum.
Affine models are valid only for weak electromagnetic fields.
Proposes that a simpler affine Lagrangian could describe gravity, electromagnetism, and dark energy.
Abstract
The Ferraris-Kijowski purely affine Lagrangian for the electromagnetic field, that has the form of the Maxwell Lagrangian with the metric tensor replaced by the symmetrized Ricci tensor, is dynamically equivalent to the metric Einstein-Maxwell Lagrangian, except the zero-field limit, for which the metric tensor is not well-defined. This feature indicates that, for the Ferraris-Kijowski model to be physical, there must exist a background field that depends on the Ricci tensor. The simplest possibility, supported by recent astronomical observations, is the cosmological constant, generated in the purely affine formulation of gravity by the Eddington Lagrangian. In this paper we combine the electromagnetic field and the cosmological constant in the purely affine formulation. We show that the sum of the two affine (Eddington and Ferraris-Kijowski) Lagrangians is dynamically inequivalent to…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
